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A 12.4 day periodicity in a close binary system after a supernova

A 12.4 day periodicity in a close binary system after a supernova

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2876759320

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

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Scope and Contents

Contents

Neutron stars and stellar-mass black holes are the remnants of massive star explosions. Most massive stars reside in close binary systems, and the interplay between the companion star and the newly formed compact object has been theoretically explored, but signatures for binarity or evidence for the formation of a compact object during a supernova...

Alternative Titles

Full title

A 12.4 day periodicity in a close binary system after a supernova

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Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2876759320

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2876759320

Other Identifiers

E-ISSN

2331-8422

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